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  • American Geophysical Union (AGU)  (29)
  • English  (29)
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  • American Geophysical Union (AGU)  (29)
Language
  • English  (29)
  • 1
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 1980
    In:  Geophysical Research Letters Vol. 7, No. 5 ( 1980-05), p. 305-308
    In: Geophysical Research Letters, American Geophysical Union (AGU), Vol. 7, No. 5 ( 1980-05), p. 305-308
    Abstract: We have investigated the possibility of removing particles from Io by interactions with the Jovian magnetosphere. We find that dust grains of about 0.1 µm radius will rapidly become charged if exposed to the ambient Jovian plasma. For particles this size in Io's volcanic plumes, the Lorentz force can overcome Io's gravity and these particles can escape. Escaping dust will be controlled by the topology of the magnetosphere and we suggest that Io derived dust may be an important source of erosive impacts on large Jovian ring particles and destructive collisions with small particles. The ring particles themselves will interact with the Jovian plasma and we suggest that coulomb scattering of plasma particles by charged dust grains may produce a plasma gap or void in the vicinity of the rings.
    Type of Medium: Online Resource
    ISSN: 0094-8276 , 1944-8007
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 1980
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    detail.hit.zdb_id: 7403-2
    SSG: 16,13
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  • 2
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 2000
    In:  Eos, Transactions American Geophysical Union Vol. 81, No. 51 ( 2000-12-19), p. 627-627
    In: Eos, Transactions American Geophysical Union, American Geophysical Union (AGU), Vol. 81, No. 51 ( 2000-12-19), p. 627-627
    Abstract: The last two of the large planetary probes of the National Aeronautic and Space Administration and the European Space Agency will rendezvous at the end of the year at Jupiter. At that time, Galileo, which has been exploring Jupiter since the end of 1995, and Cassini, which is on its way to Saturn, will simultaneously observe the Jovian system with U.S.‐ and European‐built instruments. Cassini will monitor the upstream solar wind conditions and image the magnetosphere and the moons of Jupiter; simultaneously, Galileo will report on the changing plasma conditions from inside the magnetosphere (Figure 1). This is a unique opportunity that will benefit the whole community studying the complex behavior of the Jovian system. The geometry of the two spacecraft during the encounter is especially fortunate for dust measurements, which will greatly enhance our understanding of the Jovian dust environment and the science return for both Galileo and Cassini at Jupiter. These measurements will also provide an opportunity to cross‐calibrate the dust instruments; this will be useful in the future analysis of the Cassini dust observations at Saturn.
    Type of Medium: Online Resource
    ISSN: 0096-3941 , 2324-9250
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 2000
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    detail.hit.zdb_id: 2118760-5
    detail.hit.zdb_id: 240154-X
    SSG: 16,13
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  • 3
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 2003
    In:  Geophysical Research Letters Vol. 30, No. 2 ( 2003-01)
    In: Geophysical Research Letters, American Geophysical Union (AGU), Vol. 30, No. 2 ( 2003-01)
    Type of Medium: Online Resource
    ISSN: 0094-8276
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 2003
    detail.hit.zdb_id: 2021599-X
    detail.hit.zdb_id: 7403-2
    SSG: 16,13
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  • 4
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 1997
    In:  Geophysical Research Letters Vol. 24, No. 17 ( 1997-09-01), p. 2175-2178
    In: Geophysical Research Letters, American Geophysical Union (AGU), Vol. 24, No. 17 ( 1997-09-01), p. 2175-2178
    Type of Medium: Online Resource
    ISSN: 0094-8276
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 1997
    detail.hit.zdb_id: 2021599-X
    detail.hit.zdb_id: 7403-2
    SSG: 16,13
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  • 5
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 1999
    In:  Journal of Geophysical Research: Planets Vol. 104, No. E10 ( 1999-10-25), p. 24111-24120
    In: Journal of Geophysical Research: Planets, American Geophysical Union (AGU), Vol. 104, No. E10 ( 1999-10-25), p. 24111-24120
    Abstract: The satellite Enceladus is obviously the main source of Saturn's E ring. Up to now, different mechanisms of how particles are delivered from this satellite have been suggested. In this paper, we try to answer the question of whether these different launch processes can be distinguished by the cosmic dust analyzer (CDA) aboard the Cassini spacecraft. To this aim, the dynamics of dust particles just launched from the surface of Enceladus is studied numerically. We have integrated the equations of motion for a wide range of initial conditions including ejecta from interplanetary and E ring impactors onto Enceladus. According to our simulations, Cassini will encounter a significant dust stream about the time of closest approach to Enceladus. The duration and intensity of this expected enhanced impact rate onto the CDA depends on the way the particles are ejected from the satellite. The counting rate yields information about the distribution of ejecta sources on the surface of Enceladus. For instance, an anisotropy of the ejecta between the leading and the trailing hemispheres of Enceladus should be detectable, and impactors of different origin should be distinguishable. Furthermore, the vertical component of the ejecta velocities can explain the vertical extent of the E ring.
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 1999
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    SSG: 16,13
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  • 6
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 2011
    In:  Geophysical Research Letters Vol. 38, No. 24 ( 2011-12-28), p. n/a-n/a
    In: Geophysical Research Letters, American Geophysical Union (AGU), Vol. 38, No. 24 ( 2011-12-28), p. n/a-n/a
    Type of Medium: Online Resource
    ISSN: 0094-8276
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 2011
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    detail.hit.zdb_id: 7403-2
    SSG: 16,13
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  • 7
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 2014
    In:  Journal of Geophysical Research: Space Physics Vol. 119, No. 8 ( 2014-08), p. 6294-6312
    In: Journal of Geophysical Research: Space Physics, American Geophysical Union (AGU), Vol. 119, No. 8 ( 2014-08), p. 6294-6312
    Abstract: Cassini RPWS detects dust impacts as voltage pulses induced on the antennas The dust size distribution and density can be inferred from the measurements The observed dust density and size distribution are consistent with CDA results
    Type of Medium: Online Resource
    ISSN: 2169-9380 , 2169-9402
    URL: Issue
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 2014
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    detail.hit.zdb_id: 161665-1
    detail.hit.zdb_id: 3094181-7
    SSG: 16,13
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  • 8
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 2014
    In:  Journal of Geophysical Research: Space Physics Vol. 119, No. 8 ( 2014-08), p. 6019-6026
    In: Journal of Geophysical Research: Space Physics, American Geophysical Union (AGU), Vol. 119, No. 8 ( 2014-08), p. 6019-6026
    Abstract: Impact ionization was measured for spacecraft‐relevant materials Yields are smaller than predicted by certain published laws Yields do not differ strongly between materials tested at 10 km/s
    Type of Medium: Online Resource
    ISSN: 2169-9380 , 2169-9402
    URL: Issue
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 2014
    detail.hit.zdb_id: 2033040-6
    detail.hit.zdb_id: 161665-1
    detail.hit.zdb_id: 3094181-7
    SSG: 16,13
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  • 9
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 2000
    In:  Journal of Geophysical Research: Space Physics Vol. 105, No. A5 ( 2000-05), p. 10291-10297
    In: Journal of Geophysical Research: Space Physics, American Geophysical Union (AGU), Vol. 105, No. A5 ( 2000-05), p. 10291-10297
    Abstract: Identification by the Ulysses spacecraft of interstellar grains inside the planetary system provides a new window for the study of diffuse interstellar matter. Dust particles observed by Ulysses and confirmed by Galileo are more massive (≥ 10 −13 g) than the “classical” interstellar grains. Even bigger grains (≈ 10 −7 g) were observed in form of interstellar meteors. We analyze the consequences of the plentiful existence of massive grains in the diffuse interstellar medium. Astronomically observed classical interstellar grains can be described by a size distribution ranging from ∼ 5 to 250 nm in radius (∼ 10 −18 to 10 −13 g). Lifetimes of these particles, owing to mutual collisions in interstellar space, can be as short as 10 5 f years, where f = 10 to 1000, is the fraction of total lifetime to the time when grains are exposed to supernova shocks. Shattering is a source of the smallest of these grains, but grains more massive than ∼ 10 −16 g of the classical interstellar grain population are rapidly destroyed. When applying the same shattering mechanism to the more massive grains found recently, we suggest that collisions of particles bigger than ∼ 10 −15 g provide a source for smaller grains. Because massive grains couple to the interstellar gas only over large (100 to 1000 pc) length scales, the cosmic abundance ratio of gas‐to‐dust needs only to be preserved averaged over corresponding volumes of space.
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 2000
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    detail.hit.zdb_id: 161666-3
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    detail.hit.zdb_id: 161665-1
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    detail.hit.zdb_id: 3094181-7
    detail.hit.zdb_id: 3094219-6
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    detail.hit.zdb_id: 2220777-6
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    SSG: 16,13
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  • 10
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 1999
    In:  Journal of Geophysical Research: Solid Earth Vol. 104, No. B8 ( 1999-08-10), p. 17531-17549
    In: Journal of Geophysical Research: Solid Earth, American Geophysical Union (AGU), Vol. 104, No. B8 ( 1999-08-10), p. 17531-17549
    Abstract: We present a new method for the assessment of the most recent cooling and denudation rates using paramagnetic centers in quartz measured by electron spin resonance (ESR) spectroscopy. These centers have a relatively low thermal stability. For cooling rates of 40° and 1000°C Myr −1 , effective closure temperatures vary between 55° and 82°C (Ti center) and 49° and 64°C (Al center), respectively. Samples were collected from two cores that were drilled into the Eldzhurtinskiy Granite, which has an emplacement age of ∼2 Ma as measured by U/Pb analyses of zircons. One 1500 m core was taken from a drill hole into the dome of the granite, a second core of 4000 m from a drill hole at the base of the Baksan Valley. Our results yield cooling rates of between 160 and 250°C Myr −1 for the upper core and between 570° and 600°C Myr −1 for the lower core; the corresponding denudation rates are ∼2.5 (upper core) and 5.5 mm a −1 (lower core). The shape of the temperature profile of the lower core indicates recent erosion. When fitting the temperature data with a two‐dimensional heat‐transfer model, we obtain a net denudation rate of ∼10 mm a −1 and cooling rates in the range of 500°C Myr −1 , thus confirming the cooling rates estimated by ESR. However, the ESR denudation rates underestimate the erosion rate of the Baksan Valley because the geothermal gradient is not equilibrated between the surface and the depth of the annihilation temperatures, 950 and 1800 m for the Al and Ti centers, respectively. We conclude that ESR measurements of paramagnetic centers in quartz will allow the reconstruction of landscape dynamics for the past 10–1000 kyr and that in conjunction with U/Pb, fission track, and Ar/Ar analyses it will be possible to develop dynamic models for Quaternary tectonic movements.
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 1999
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    detail.hit.zdb_id: 2220777-6
    detail.hit.zdb_id: 3094197-0
    SSG: 16,13
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